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Avaroth Harindranath, Saha Institute of Nuclear Physics, Calcutta, India Dipankar Chakrabarty, Florida State University Lubo Martinovic, Institute of Physics Institute, Bratislava, Slovakia Grigorii Pivovarov, Institute for Nuclear Research, Moscow, Russia Peter Peroncik, Richard Lloyd, John R. Spence, James P. Vary, Iowa State University Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory I. Ab initio approach to quantum many-body systems II. Constituent quark models & light front 4 LC2005 - Cairns, Australia July 7-15 , 2005

Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory

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Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory. Avaroth Harindranath, Saha Institute of Nuclear Physics, Calcutta, India Dipankar Chakrabarty, Florida State University Lubo Martinovic, Institute of Physics Institute, Bratislava, Slovakia - PowerPoint PPT Presentation

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Page 1: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory

Avaroth Harindranath, Saha Institute of Nuclear Physics, Calcutta, India

Dipankar Chakrabarty, Florida State University

Lubo Martinovic, Institute of Physics Institute, Bratislava, Slovakia

Grigorii Pivovarov, Institute for Nuclear Research, Moscow, Russia

Peter Peroncik, Richard Lloyd, John R. Spence, James P. Vary,

Iowa State University

Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory

I. Ab initio approach to quantum many-body systemsII. Constituent quark models & light front 4

1+1

III. Conclusions and Outlook

LC2005 - Cairns, AustraliaJuly 7-15 , 2005

Page 2: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory

Constructing the non-perturbative theory bridge between“Short distance physics” “Long distance physics”

Asymptotically free current quarks Constituent quarksChiral symmetry Broken Chiral symmetryHigh momentum transfer processes Meson and Baryon Spectroscopy

NN interactions

H(bare operators) HeffBare transition operators Effective charges, transition ops, etc.

Bare NN, NNN interactions Effective NN, NNN interactions fitting 2-body data describing low energy nuclear dataShort range correlations & Mean field, pairing, & strong tensor correlations quadrupole, etc., correlations

BOLD CLAIM We now have the tools to accomplish this program in

nuclear many-body theory

Page 3: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory

H acts in its full infinite Hilbert Space

Heff of finite subspace

Ab Initio Many-Body Theory

Page 4: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory

H =Trel + V (a)

HA = Trel +V = [(

r p i −

r p j )

2

2mA+ Vij

i< j

A

∑ ] + VNNN

P. Navratil, J.P. Vary and B.R. Barrett, Phys. Rev. Lett. 84, 5728(2000); Phys. Rev. C62, 054311(2000)C. Viazminsky and J.P. Vary, J. Math. Phys. 42, 2055 (2001);K. Suzuki and S.Y. Lee, Progr. Theor. Phys. 64, 2091(1980);

K. Suzuki, ibid, 68, 246(1982); K. Suzuki and R. Okamoto, ibid, 70, 439(1983)

Preserves the symmetries of the full Hamiltonian:Rotational, translational, parity, etc., invariance

Effective Hamiltonian for A-ParticlesLee-Suzuki-Okamoto Method plus Cluster Decomposition

Select a finite oscillator basis space (P-space) and evaluate an - body cluster effective Hamiltonian:

Guaranteed to provide exact answers as or as .

a

a → A

P → 1

Page 5: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory

NMIN=0

NMAX=6configuration

“6h” configuration for 6Li

Page 6: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory

Select a subsystem (cluster) of a < A Fermions.

Develop a unitary transformation for a finite space,the “P-space” that generates the exact low-lying spectraof that cluster subsytem. Since it is unitary, it preservesall symmetries.

Construct the A-Fermion Hamiltonian from this a-Fermioncluster Hamiltonian and solve for the A-Fermion spectraby diagonalization.

Guaranteed to provide the full spectra as either a --> A or as P --> 1

Guide to the methodology

Page 7: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory

H (a) =(Pa +ωTω)−1/ 2(Pa + PaωTQa )Ha

Ω(QaωPa + Pa )(Pa + ωTω)−1/ 2

HaΩ k =Ek k

αQ ω αP = αQ kk∈K∑ ˆ k αP

where: ˆ k αP =Inverse{k αP }

Pa = αPP∈P∑ αP

Qa = αQQ∈Q∑ αQ

Pa +Qa ≈1a

Key equations to solve at the a-body cluster level

Solve a cluster eigenvalue problem in a very large but finite basisand retain all the symmetries of the bare Hamiltonian

Page 8: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory

Historical PerspectiveNuclei with Realistic Interactions

1985 - Exact solution of Fadeev equations (3-Fermions)1991 - Exact solution of Fadeev-Jacobovsky equations (4-Fermions)2000 - Green’s Function Monte Carlo solutions up to A = 102000 - Ab-initio solutions for A = 12 via effective operators

Present day applications with effective operators:A = 16 solved with realistic NN interactionsA = 14 solved with realistic NN and NNN interactions

Page 9: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory
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Page 13: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory

Constituent Quark Models of Exotic MesonsR. Lloyd, PhD Thesis, ISU 2003Phys. Rev. D 70: 014009 (2004)

H = T + V(OGE) + V(confinement)

Solve in HO basis as a bare H problem & study dependence on cutoff

Symmetries:Exact treatment of color degree of freedom <-- Major new accomplishmentTranslational invariance preservedAngular momentum and parity preserved

Next generation:More realistic H fit to wider range of mesons and baryonsSee preliminary results below.

Beyond that generation:Heff derived from QCD using light-front quantization

Page 14: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory

Nmax/2

Mas

s(M

eV)

Page 15: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory
Page 16: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory

Burning issues

Demonstrate degeneracy - Spontaneous Symmetry BreakingTopological features - soliton mass and profile (Kink, Kink-Antikink)

Quantum modes of kink excitationPhase transition - critical coupling, critical exponent and

the physics of symmetry restorationRole and proper treatment of the zero mode constraint

Chang’s Duality

4 in 1+1 Dimensions

Page 17: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory

4 in 1+1 DimensionsDLCQ with Coherent State Analysis

A. Derive the Hamiltonian and quantize it on the light front, investigate coherent state treatment of vacuum A. Harindranath and J.P. Vary, Phys Rev D36, 1141(1987)

B. Obtain vacuum energy as well as the mass and profile functions of soliton-like solutions in the symmetry-broken phase:

PBC: SSB observed, Kink + Antinkink ~ coherent state!Chakrabarti, Harindranath, Martinovic, Pivovarov and Vary,Phys. Letts. B to be published; hep-th/0310290.

APBC: SSB observed, Kink ~ coherent state!Chakrabarti, Harindranath, Martinovic and Vary, Phys. Letts. B582, 196 (2004); hep-th/0309263

C. Demonstrate onset of Kink Condensation:Chakrabarti, Harindranath and Vary, Phys. Rev. D71, 125012(2005); hep-th/0504094

Page 18: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory

Lagrangian density

=12

(∂μφ∂μφ + μ 2φ2 ) −λ4!

φ 4

Hamiltonian quantized in light front coordinates with, for example, anti - periodic boundary conditions:H = H 0 + H1 + H2

H0 = −μ 2 1n

an+

n =1/2

K

∑ an

H1 =λ4π

1N kl

21

Nmn2

ak+al

+aman

klmnk ≤l ,m ≤n

K

∑ δm + n,k +l

H2 =λ

4π1

N lmn2 [

ak+alaman + an

+am+ al

+ak

klmnk ,l ≤m ≤ n

K

∑ ]δ k,m + n+ l

N kl2 =1, k ≠ l N lmn

2 =1,l ≠ m ≠ n = 2!,k = l = 2!, l = m ≠ n,l ≠ m = n = 3!,l = m = nwhere all indecies are half odd integers.

L

Page 19: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory

nkk∑ k = K

H ψ i = E i ψ i

Fully covariant mass - squared spectra emergesM i

2 = KE i

Must extrapolate to the continuum limit, K - > ∞

At finite K, results are compared with results from a constrained variational treatment based on the coherent state ansatz of J.S. Rozowski and C.B. Thorn, Phys. Rev. Lett. 85, 1614 (2000).

Set up a normalized and symmetrized set of basis states, where, with representing the number of bosons with light front momentum k:

nk

Page 20: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory

DLCQ matrix dimension in even particle sector (APBC)

K Dimension16 33632 1421940 6724345 16549850 38925355 88096260 1928175

Page 21: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory

χ(n) = K an+an K

Normalized:

nn∑ χ (n) = K

Light cone momentum fraction:x = n / K

Light front momentum probability density in DLCQ:

Compares favorably with results from a constrainedvariational treatment based on the coherent state

Page 22: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory
Page 23: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory

M02 = E0vK + M kinkK

2

=> E0 = M02 / K = E0v + M kinkK

Note:φ → −φ symmetry=> Decoupling of even and odd boson sectors=> Exact degeneracy only in the K → ∞ limit

Extract the Vacuum energy density and Kink Mass

All results to date are in the broken phase:

μ 2 = −1

Define a Ratio = [M2even - M2

odd]/ [Vac Energy Dens]2

Page 24: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory

PBC

Page 25: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory

fit range

Page 26: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory

Vacuum Energy

Classical DLCQ-APBC

DLCQ-PBCzero modes?

0.5 -37.70 -37.81(7) -37.90(4)

1.0 -18.85 -18.71(5) -18.97(2)

1.25 -15.08 -14.91(5) 15.19(5)

Page 27: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory

Soliton Mass

Classical Semi-Classical

DLCQ-APBC

DLCQ-PBCzero modes?

0.5 11.31 10.84 11.6(2) 11.26(4)

1.00 5.657 5.186 5.22(8) 5.563(7)

1.25 4.526 4.054 4.07(6) 4.43(4)

Page 28: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory

Fourier Transform of the Soliton (Kink) Form Factor Ref: Goldstone and Jackiw

φc (x− − a) = dq+ exp −i2

q+a ⎧ ⎨ ⎩

⎫ ⎬ ⎭−∞

∫ K + q+ Φ(x −) K

Evaluated within DLCQ choosing a = 0:

=14πl

l =12

,32

,52

,...

∑ K ± l ale−lπ

x −

L + al+e

lπx −

L ⎧ ⎨ ⎩

⎫ ⎬ ⎭ K

Note: Issue of the relative phases - fix arbitrary phases viaguidance of the the coherent state analysis:

Sign K + l al+ K{ } = +

Sign K − l al K{ } = −

Cancellation of imaginary terms and vacuum expectation value, ,are non-trivial tests of resulting kink structure.

φ

Page 29: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory

Quantum kink (soliton) in scalar field theory at = 1

Page 30: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory

Can we observe a phase transition in ?

1+14

How does a phase transition develop as a function of increased coupling?

What are the observables associated with a phase transition?

What are its critical properties (coupling, exponent, …)?

Page 31: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory
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Page 37: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory

Continuum limit of the critical coupling

Page 38: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory
Page 39: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory
Page 40: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory

Light front momentum distribution functions

Page 41: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory
Page 42: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory

What is the nature of this phase transition?

(1) Mass spectroscopy changes(2) Form factor character changes -> Kink condensation signal(3) Parton distribution changes

Page 43: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory

QCD applications in the -link approximation for mesons

qq + qq

S. Dalley and B. van de Sande, Phys. Rev. D67, 114507 (2003); hep-ph/0212086

D. Chakrabarti, A. Harindranath and J.P. Vary, Phys. Rev. D69, 034502 (2004); hep-ph/0309317

DLCQ for longitudinal modes and a transverse momentum lattice

Adopt QCD Hamiltonian of Bardeen, Pearson and Rabinovici Restrict the P-space to q-qbar and q-qbar-link configurations Does not follow the effective operator approach (yet) Introduce regulators as needed to obtain cutoff-independent spectra

Page 44: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory

Full q-qbar comps q-qbar-link comps

Lowest state

Fifth state

Page 45: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory

Conclusions

• Similarity of “two-scale” problems in quantum systems with many degrees of freedom• Ab-initio theory is a convergent exact method for solving many-particle Hamiltonians• Two-body cluster approximation (easiest) suitable for many observables• Method has been demonstrated as exact in the nuclear physics applications• Quasi-exact results for 1+1 scalar field theory obtained • Non-perturbative vacuum expectation value (order parameter)• Kink mass & profile obtained• Critical properties (coupling, exponent) emerging• Evidence of Kink condensation obtained• Sensitivity to boundary conditions needs further study• Role of zero modes yet to be fully clarified (Martinovic talk tomorrow)• Advent of low-cost parallel computing has made new physics domains accessible: algorithm improvements have achieved fully scalable and load-balanced codes.

Page 46: Coherent States and Spontaneous Symmetry Breaking in Light Front Scalar Field Theory

Future Plans

Apply LF-transverse lattice and basis functions to qqq systems (Stan Brodsky’s talk)

Investigate alternatives Effective Operator methods (Marvin Weinstein’s - CORE)

Improve semi-analytical approaches for accelerating convergence (Non-perturbative renormalization approaches - for discussion)